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The WAGGS project - I. The WiFeS Atlas of Galactic Globular cluster Spectra

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arxiv 1703.07397 v1 pith:QR4235QD submitted 2017-03-21 astro-ph.GA

The WAGGS project - I. The WiFeS Atlas of Galactic Globular cluster Spectra

classification astro-ph.GA
keywords globularclustersmilkyspectraclusterintegratedwifesatlas
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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We present the WiFeS Atlas of Galactic Globular cluster Spectra, a library of integrated spectra of Milky Way and Local Group globular clusters. We used the WiFeS integral field spectrograph on the Australian National University 2.3 m telescope to observe the central regions of 64 Milky Way globular clusters and 22 globular clusters hosted by the Milky Way's low mass satellite galaxies. The spectra have wider wavelength coverage (3300 {\AA} to 9050 {\AA}) and higher spectral resolution (R = 6800) than existing spectral libraries of Milky Way globular clusters. By including Large and Small Magellanic Cloud star clusters, we extend the coverage of parameter space of existing libraries towards young and intermediate ages. While testing stellar population synthesis models and analysis techniques is the main aim of this library, the observations may also further our understanding of the stellar populations of Local Group globular clusters and make possible the direct comparison of extragalactic globular cluster integrated light observations with well understood globular clusters in the Milky Way. The integrated spectra are publicly available via the project website.

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  1. Cosmic CORALS: Timing the Universe with high-z star clusters

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    Star clusters at z=9.6 combined with local globular cluster ages give H0=70(+27,-16) km/s/Mpc and Omega_m=0.33(+0.37,-0.21), with a forecast that ~300 clusters could reach 4% precision.